The occurrence rate of type III solar bursts in the frequency range 4.9 MHz to 30 kHz is analyzed as a function of burst intensity and burst arrival direction. We find that (a) the occurrence rate of bursts falls off with increasing flux, S, according to the power law S -1s, and (b) the distribution
On the spatial directivity of solar radio bursts
โ Scribed by I. E. Pogodin; A. G. Stupishin; K. Shibasaki
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 362 KB
- Volume
- 167
- Category
- Article
- ISSN
- 0038-0938
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